Astronomers have discovered a mysterious little dwarf planet which they believe is covered in ice and may sport the wispy remnants of an atmosphere. The planet, nicknamed "Snow White", lies outside Neptune and is orbiting the sun as part of the Kuiper belt -- the ring of icy bodies that orbit the sun beyond Neptune. Officially known as 2007 OR10, it is actually red, half of its surface is covered by water ice that probably spewed from ancient cryovolcanoes, researchers said. Read more
Astronomers Find Ice and Possibly Methane on Snow White, a Distant Dwarf Planet
Astronomers at the California Institute of Technology (Caltech) have discovered that the dwarf planet 2007 OR10 - nicknamed Snow White - is an icy world, with about half its surface covered in water ice that once flowed from ancient, slush-spewing volcanoes. The new findings also suggest that the red-tinged dwarf planet may be covered in a thin layer of methane, the remnants of an atmosphere that's slowly being lost into space. Read more
Title: The surface composition of large Kuiper belt object 2007 OR10 Authors: M.E. Brown, A.J. Burgasser, W.C. Fraser
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice. While most objects in the Kuiper belt with water ice absorption this prominent have the optically neutral colours of water ice, 2007 OR10 is among the reddest Kuiper belt objects known. One other large Kuiper belt object -- Quaoar -- has similar red colouring and water ice absorption, and it is hypothesized that the red coloration of this object is due to irradiation of the small amounts of methane able to be retained on Quaoar. 2007 OR10, though warmer than Quaoar, is in a similar volatile retention because it is sufficiently larger that its stronger gravity can still retain methane. We propose, therefore, that the red coloration on 2007 OR10 is also caused by the retention of small amounts of methane. Positive detection will require spectra of methane on 2007 OR10 will require spectra with higher signal-to-noise. Models for volatile retention on Kuiper belt objects appear to continue to do an excellent job reproducing all of the available observations.
Kuiper Belt Object (225088) 2007 OR10 is a trans-Neptunian object with an absolute magnitude of 1.7. This qualifies it as one of the largest dwarf-planet candidates: Mike Brown estimates that it is between Sedna and Quaoar in size. Mike Brown's discovery team has nicknamed the object "Snow White", as it would have to be very large or very bright to be detected by their survey. It is currently the largest known Solar System object without an official name. Read more
The survey that found Snow White was specifically looking for quite distant things like Sedna; things that would help us better understand the beginning of the solar system. Snow White, we finally learned, was not like Sedna at all. It was just a normal Kuiper belt object found slightly far away. Bigger than most, but otherwise, as far as we knew, unremarkable. Read more
(225088) 2007 OR10 is a Trans-Neptunian object with an absolute magnitude of 1.9. This qualifies it as one of the largest dwarf planet candidates: Brown estimates that it is between Sedna and Quaoar in size. Mike Brown's discovery team has nicknamed the object "Snow White", as it would have to be very large or very bright to be detected by their survey. The Trans-Neptunian Object (225088) 2007 OR10 was discovered on the 17th July, 2007.